Disk-resolved spectral characteristics of Ganymede and Callisto

Details Disk-resolved spectral characteristics of Ganymede and Callisto Disk-resolved spectral characteristics of Ganymede and Callisto

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..293d&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 293.

Computer Science

1

Ganymede, Callisto, Spectral Signatures, Satellite Surfaces, Planetary Composition, Grain Size, Minerals, Spectrum Analysis, Spectral Resolution

Scientific paper

Three different kinds of spectral signatures for ice and nonice
components found on Ganymede and Callisto are discussed. The reasons for
this, possibly material differences or grain size effects, are
addressed.

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